Mathematics – Logic
Scientific paper
Jan 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001iaus..204..413m&link_type=abstract
The Extragalactic Infrared Background and its Cosmological Implications, Proceedings of IAU Symposium #204, held 15-18 August 20
Mathematics
Logic
2
Scientific paper
By consistently connecting chemical and spectrophotometric evolution we are able to include the effect of dust absorption. The time and redshift evolution of extinction is based on the evolution of the gas content and metallicity. We present our evolutionary synthesis models which include dust absorption to analyse the UV emission in various galaxy types. We are able to predict E(B-V) for different galaxy types as a function of redshift. We further use these models to explore the range of metallicities in normal and starbursting galaxies and the metallicity distribution of the stellar population. Comparing our model SED's with templates from Kennicutt's and Kinney et al.'s atlas we show detailed agreement with integrated spectra of galaxies and point out the importance of aperture effects. Combined with a cosmological model we show the differences in the evolutionary and k-corrections comparing models with and without dust.
Alvensleben Uta Fritze--v.
Calzetti Daniela
Fricke Klaus J.
Möller Claudia S.
No associations
LandOfFree
Metallicities and Dust in High-z Galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Metallicities and Dust in High-z Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Metallicities and Dust in High-z Galaxies will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1362708